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We present the results of a program to acquire photometry for eighty-six late-M, L, and T dwarfs using the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. We examine the behavior of these cool dwarfs in various color-color and…

Ultra-cool white dwarfs are among the oldest stellar remnants in the Universe. Their efficient gravitational settling and low effective temperatures are responsible for the smooth spectra they exhibit. For that reason, it is not possible to…

Solar and Stellar Astrophysics · Physics 2020-04-08 M. C. Lam , N. C. Hambly , N. Lodieu , S. Blouin , E. J. Harvey , R. J. Smith , M. C. Galvez-Ortiz , Z. H. Zhang

We present initial results of an all-sky search for late-type dwarfs within 20 pc of the Sun using the New Luyten Two-Tenths (NLTT) catalog cross-referenced with the 2-Micron All Sky Survey (2MASS) database. The results were obtained with…

Astrophysics · Physics 2009-11-07 Kelle L. Cruz , I. Neill Reid

We present the discovery of three late type (>T4) brown dwarfs, including a probable Y dwarf, in the WFC3 Infrared Spectroscopic Parallels (WISP) Survey. We use the G141 grism spectra to determine the spectral types of the dwarfs and derive…

We report an attempt to interpret the spectra of L and T dwarfs with the use of the Unified Cloudy Model (UCM). For this purpose, we extend the grid of the UCMs to the cases of log g = 4.5 and 5.5. The dust column density relative to the…

Astrophysics · Physics 2009-11-10 Takashi Tsuji , Tadashi Nakajima , Kenshi Yanagisawa

We present observations of the T8 dwarf 2MASS 0415-0935 with JWST's NIRSpec spectrograph using the G395H grating ($\sim$ 2.87 - 5.14 $\mu$m). We perform the first atmospheric retrieval analysis at the maximum spectral resolution of NIRSpec…

We have obtained near-infrared images and spectra of three blue compact dwarf galaxies of intermediate sub-solar metallicity Tol~35, Tol~3 and UM 462. This work is part of a larger project aimed to study the star formation and the stellar…

Astrophysics · Physics 2009-11-07 L. Vanzi , L. K. Hunt , T. X. Thuan

Benchmark brown dwarfs are those objects for which fiducial constraints are available, including effective temperature, parallax, age, metallicity. We searched for new cool brown dwarfs in 186 sq.deg. of the new area covered by the data…

Solar and Stellar Astrophysics · Physics 2015-05-18 B. Goldman , S. Marsat , T. Henning , C. Clemens , J. Greiner

We present the serendipitous discovery of an L subdwarf, 2MASS J06164006-6407194, in a search of the Two Micron All Sky Survey for T dwarfs. Its spectrum exhibits features indicative of both a cool and metal poor atmosphere including a…

Solar and Stellar Astrophysics · Physics 2014-11-18 M. C. Cushing , D. Looper , A. J. Burgasser , J. D. Kirkpatrick , J. Faherty , K. Cruz , A. Sweet , R. E. Sanderson

Aims: A near-infrared study of the main ionizing star of the ultracompact HII region G23.96+0.15 (IRAS 18317-0757) is presented, along with a re-evaluation of the distance to this source, and a re-assessment of H- and K-band classification…

Astrophysics · Physics 2009-11-13 Paul A Crowther , James P Furness

We aim to provide a detailed characterization of near-infrared spectra for young LT brown dwarfs, including robust spectral typing, calibrating spectral indices, identifying possible binaries, and selecting suitable spectral standards. We…

Solar and Stellar Astrophysics · Physics 2024-05-29 L. Piscarreta , K. Mužić , V. Almendros-Abad , A. Scholz

SDSS J080531.84+481233.0 is a peculiar L-type dwarf that exhibits unusually blue near-infrared and mid-infrared colors and divergent optical (L4) and near-infrared (L9.5) spectral classifications. These peculiar spectral traits have been…

Astrophysics · Physics 2009-06-23 Adam J. Burgasser

We test state-of-the-art model atmospheres for young very low-mass stars and brown dwarfs in the infrared, by comparing the predicted synthetic photometry over 1.2-24 {\mu}m to the observed photometry of M-type spectral templates in…

Solar and Stellar Astrophysics · Physics 2015-05-27 Jonathan Tottle , Subhanjoy Mohanty

We report the discovery of a resolved (0".9) substellar companion to a member of the 1-5 Myr Taurus star-forming region. The host star (2M0437) is a single mid-M type ($T_{eff}\approx$3100K) dwarf with a position, space motion, and…

We present the first high-resolution (R ~ 31,000) spectra of the cool sdL 2MASS0532, and what was originally identified as an early-type L subdwarf (sdL) LSR1610-0040. Our work, in combination with contemporaneous work by Cushing and Vacca,…

Astrophysics · Physics 2008-11-26 Ansgar Reiners , Gibor Basri

We present YJHK photometry, or a subset, for the six Y dwarfs discovered in WISE data by Cushing et al.. The data were obtained using NIRI on the Gemini North telescope. We also present a far-red spectrum obtained using GMOS-North for…

Solar and Stellar Astrophysics · Physics 2015-06-12 S. K. Leggett , Caroline V. Morley , M. S. Marley , D. Saumon , Jonathan J. Fortney , Channon Visscher

Y dwarfs represent the coldest class of brown dwarfs, with effective temperatures below 500K, and provide unique analogues to cold giant exoplanets. We present a large compilation of uniform near-infrared photometry from the Hubble Space…

This work presents the first results of near-infrared (NIR) counterparts of ultraluminous X-ray sources (ULXs) in the case of NGC 1672 by using James Webb Space Telescope (JWST) observations. Through advanced astrometry, unique counterparts…

High Energy Astrophysical Phenomena · Physics 2023-10-31 Sinan Allak

We present Herschel and XMM-Newton observations of ULASJ1234+0907 ($z=2.503$), the reddest broad-line Type 1 quasar currently known with (i-K)>7.1. Herschel observations indicate that the quasar host is a hyperluminous infrared galaxy…

Astrophysics of Galaxies · Physics 2019-08-19 Manda Banerji , Andy Fabian , Richard McMahon

We present 11 candidate late-type companions to nearby stars identified with data from the Wide-field Infrared Survey Explorer (WISE) and the Two Micron All-Sky Survey (2MASS). Eight of the candidates are likely to be companions based on…